Results 31 to 40 of about 4,003,229 (276)

New Candidate Massive Clusters from 2MASS [PDF]

open access: yes, 2013
Massive stars are important for the evolution of the interstellar medium. The detailed study of their properties (such as mass loss, rotation, magnetic fields) is enormously facilitated by samples of these objects in young massive galactic star clusters.
Dirk Froebrich, Froebrich, Dirk
core   +1 more source

Observational Evidence of the Merging of Filaments and Hub Formation in G083.097+03.270

open access: yesThe Astrophysical Journal, 2023
We uncover a hub–filament system correlated with massive young stellar associations in G083.097+03.270. Diagnosed with simultaneous ^12 CO, ^13 CO, and C ^18 O line observations, the region is found to host two distinct and elongated filaments having ...
Alik Panja   +6 more
doaj   +1 more source

Young Massive Clusters [PDF]

open access: yesProceedings of the International Astronomical Union, 2007
AbstractOver the past ten years, there has been a revolution in our understanding of massive young stellar clusters in the Galaxy. Initially, there were no known examples having masses >104, yet we now know that there are at least a half dozen such clusters in the Galaxy.
openaire   +2 more sources

The Formation and Early Evolution of Young Massive Clusters [PDF]

open access: yes, 2014
24 pages, 1 figure. Accepted for publication as a chapter in Protostars and Planets VI, University of Arizona Press (2014), eds. H. Beuther, R. Klessen, C.
S. N. Longmore   +9 more
openaire   +3 more sources

LRG1 Drives Pathological Angiogenesis by Disrupting Neutrophil Mitochondrial Homeostasis in Bladder Cancer. [PDF]

open access: yesAdv Sci (Weinh)
In bladder cancer, LRG1 binds to ANXA2 to trigger mitochondrial ROS‐dependent NETosis. This pathogenic cascade actively uncouples endothelial‐mural cell interactions, driving profound vascular destabilization. Consequently, targeting the LRG1‐ANXA2 axis attenuates the neutrophil burden and induces structural vascular normalization, offering a powerful ...
Chen D   +8 more
europepmc   +2 more sources

Formation of Very Young Massive Clusters and Implications for Globular Clusters [PDF]

open access: yes, 2017
49 pages, 18 figures, 4 tables. Review chapter to be published in The Origin of Stellar Clusters, ed. S. Stahler (Springer)
Banerjee, Sambaran, Kroupa, Pavel
openaire   +2 more sources

Massive Young Clusters [PDF]

open access: yes, 2005
In the last decade we have come to realize that the traditional classification of stellar clusters into open and globular clusters cannot be easily extended beyond the realm of the Milky Way, and that even for our Galaxy it is not fully valid. The main failure of the traditional classification is the existence of Massive Young Clusters (MYCs), which ...
openaire   +2 more sources

To Be or Not to Be: Alicante-8, a Cluster or Not?

open access: yesThe Astronomical Journal, 2023
Recent surveys have uncovered new young massive clusters that host dozens of red supergiants (RSGs) near the inner Galaxy. However, many of them have still not been fully studied. Using Very Large Telescope/X-shooter near-infrared spectra, we present the
Randa Asa’d   +5 more
doaj   +1 more source

Structural Properties of Massive Young Clusters [PDF]

open access: yesThe Astrophysical Journal, 2001
We have retrieved multicolor WFPC2/HST data from the STScI archive for 27 nearby Massive (>= 3x10^4 M_Sun) Young (< 20 Myr) star Clusters (MYCs). The data represents the most-complete-to-date sample of clearly resolved MYCs. We have analyzed their structural properties and have found that they can be classified as either Super Star Clusters (SSCs)
Maíz-Apellániz, Jesús   +2 more
openaire   +2 more sources

Young massive star clusters in M51 [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2002
A search for young massive star clusters (YMCs) in the nearby face-on spiral galaxy M51 (NGC 5194) has been carried out using UBV CCD images from the prime focus camera on the Lick 3 meter Shane telescope. The YMC population is found to be quite rich with a specific U-band luminosity T_L(U) = 1.4, consistent with the high current star formation rate of
openaire   +3 more sources

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